The optical properties of CsPbBr3 are studied with temperature dependent spectroscopic techniques. The samples are obtained from a method that has 10 % Pb waste compared with conventional ones. The dependence with temperature between 30 K and room temperature of the optical transmittance and photoluminescence is measured. Near bandgap optical properties are governed by structures originated in free excitons. Using the Elliott model for excitonic absorption, the dependence with temperature of bandgap energy and exciton binding energy are obtained. Both increase with temperature increase. Also, the width of the excitonic absorption and the inter-band absorption, which is assimilated to Urbach energy, were studied. Several models are used to extract parameters from these data. The excitonic absorption width follows the Segall model giving an exciton optical phonon interaction as the dominant term at room temperature. From several fittings, an effective optical phonon energy between 23 and 32 meV is obtained. The Urbach energy at 30 K reaches 10 meV which is related to a good crystalline quality of the samples. Several experimental results show that the origin of the photoluminescence is produced by direct recombination of free excitons. The first one is the similarity of the temperature dependence of photoluminescence width with the one of excitonic absorption. The second one is based in the activation energies obtained from the dependence of the integrated photoluminescence with temperature, one of which coincides with Excitonic Biding Energy. The third one is related to the dependence of the Stokes Shift with temperature which corresponds to the Gurioli model of excitonic thermalization. The last one comes from the dependence of the time resolved photoluminescence. Using rate equations, a radiative and non-radiative monomolecular time constant between 32 and 50 ns and an exciton-exciton annihilation rate constant between 1.0 and 6.0 × 10−7 cm3/s are obtained.
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